CORDIS Project
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The ISM-FLOW project aims to visualize the gas flow in the local Milky Way in three dimensions, utilizing data from the ESA Gaia mission and near-infrared observations. This research will enhance understanding of star formation and the dynamics of interstellar gas structures, challenging traditional views of the galaxy…
The current model for the structure of the local Milky Way is in crisis.
Data from the ESA Gaia mission has overthrown the 150-year-old paradigm for the gas distribution in the local Milky Way, a 500 pc ring known as Gould’s Belt.
In the newly emerging view, local star-forming regions are connected by lower-density gas.
They are part of a new organizational unit: undulating, coherent, and linear Galactic-scale gas structures.
What is the origin of these kpc-long structures, how do star-forming r…
UNIVERSITAT WIEN
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